Some dynamical effects expected from the motion of galaxies through a gaseous medium

Details Some dynamical effects expected from the motion of galaxies through a gaseous medium Some dynamical effects expected from the motion of galaxies through a gaseous medium

Feb 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975sva....18..426z&link_type=abstract

(Astronomicheskii Zhurnal, vol. 51, July-Aug. 1974, p. 721-723.) Soviet Astronomy, vol. 18, Jan.-Feb. 1975, p. 426, 427. Transl

Astronomy and Astrophysics

Astronomy

10

Celestial Mechanics, Dynamic Characteristics, Galactic Structure, Intergalactic Media, Interstellar Gas, Astronomical Photography, Hydrogen, Spiral Galaxies, Virgo Galactic Cluster

Scientific paper

It is shown that the motion of galaxies in the intergalactic medium may lead to partial disruption of the interstellar gas layer and to gas losses in the peripheral regions of the galaxies. As a result, there may arise: an HI deficiency of the type apparently occurring in the galaxies of the Virgo cluster; a color excess which, according to Holmberg (1964), is characteristic of some spiral galaxies in Virgo; and a characteristic dust layer asymmetry, as observed in some individual galaxies.

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